As soluções de buracos negros: 1916-1965
DOI:
https://doi.org/10.47456/Cad.Astro.v4n1.39861Palavras-chave:
estrelas invisíveis, buracos negros, Schwarzschild, Reissner-Nordström, Kerr, Newman, extensões analíticas, massas pontuaisResumo
Historicamente, as primeiras soluções da relatividade geral não foram reconhecidas como soluções de buracos negros. Elas foram, a princípio, idealizadas para descrever o campo gravitacional de objetos massivos esfericamente simétricos, como o Sol ou o elétron. Neste artigo, vamos apresentar as soluções de buracos negros em seu contexto histórico e mostrar como a nossa compreensão sobre o universo mudou à medida que desvendamos propriedades fundamentais sobre estes campos gravitacionais. O objetivo é apresentar uma introdução histórica sobre a relatividade geral e buracos negros, focada na teoria de gravitação e suas interpretações, como apoio didático para aqueles que pretendem iniciar os estudos sobre o tema.
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